A large number of evidences have been provided in the favor of the
accelerated expansion of the universe by Type Ia supernovae [1]}, Cosmic Microwave
Background (CMB) [2]}, weak lenseing [3]}, Large Scale Structures [4]}
and integrated Sachs-Wolfe effect [5]}. It is postulated that there exist a component
in the universe which has negative pressure is responsible for the accelerated expansion of
the universe, called Dark Energy (DE). The most familiar candidate of DE model is cosmological
constant \(\Lambda \)  which satisfy the cosmological observations [6]} but fails to resolve
the fine tuning problem and cosmic coincidence [7]}. In literature, there are many DE models
such as an evolving canonical scalar field [8]} quintessence, the phantom energy [9]},
quintom energy [10]} and so forth.
